Q89775716
classical Cepheid variable star in the constellation Cepheus
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Q89775716
Summary
Q89775716 is a classical Cepheid variable[1].
Key Facts
- Q89775716's instance of is recorded as classical Cepheid variable[2].
- Q89775716's constellation is recorded as Cepheus[3].
- Q89775716's spectral class is recorded as F8[4].
- Q89775716's catalog code is recorded as TYC 3995-1462-1[5].
- Q89775716's catalog code is recorded as AN 223.1935[6].
- Q89775716's catalog code is recorded as CSI+57-22270[7].
- Q89775716's catalog code is recorded as GCRV 14135[8].
- Q89775716's catalog code is recorded as GSC 03995-01462[9].
- Q89775716's catalog code is recorded as HIC 110964[10].
- Q89775716's catalog code is recorded as HIP 110964[11].
- Q89775716's catalog code is recorded as SV* SVS 572[12].
- Q89775716's catalog code is recorded as 2MASS J22285006+5812393[13].
- Q89775716's catalog code is recorded as WEB 19868[14].
- Q89775716's catalog code is recorded as Gaia DR2 2007997408188526336[15].
- Q89775716's catalog code is recorded as AK Cep[16].
- Q89775716's type of variable star is recorded as classical Cepheid variable[17].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.53'}[18].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.17'}[19].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.656'}[20].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.463'}[21].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.888'}[22].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.700'}[23].
- Q89775716's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.6877'}[24].
- Q89775716's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2648'}[25].
- Q89775716's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-55.00'}[26].
Body
Definition and Type
Q89775716's instance of is recorded as classical Cepheid variable[2].